Difference of Photometric Properties between Regular and Nonregular Miras in the Magellanic Clouds

Mira variables are asymptotic giant-branch pulsating stars with long pulsation periods and large amplitudes in optical bands. By applying the random forest algorithm to the I-band light curves for the Miras in the Magellanic Clouds, we have classified these Miras into regular Miras and nonregular Mi...

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Bibliographic Details
Main Authors: Ngeow, C.-C (Author), Ou, J.-Y (Author)
Format: Article
Language:English
Published: American Astronomical Society 2022
Online Access:View Fulltext in Publisher